In [1]:
import numpy as np
import matplotlib.pyplot as plt
import scipy.special as spec
import pandas as pd
from astropy.io import ascii
import scipy.stats as stats
from ipywidgets import FloatProgress
from IPython.display import display
import sys
sys.path.insert(0, '..')
import dr25Models as funcModels
In [2]:
def drawHeatMap(dataArray, imageSize, x, y, nData=[], colorBarLabel="", textOn=True, forceInt=True):
dx = x[(1,0)] - x[(0,0)];
dy = y[(0,1)] - y[(0,0)];
extent = [x[(0,0)], x[(-1,0)]+dx,y[(0,0)],y[(0,-1)]+dy];
plt.figure(figsize=imageSize);
# fig, ax = plt.subplots(figsize=imageSize);
ax = plt.gca()
da = np.transpose(dataArray);
# im = ax.imshow(da, extent = extent, origin='lower');
im = ax.imshow(da, extent = extent, origin='lower', cmap="Greys");
ax.set_aspect(10);
if len(nData) == 0:
nData = np.ones(dataArray.shape)
# ax.imshow(da, origin='lower');
arrayShape = da.shape;
minda = np.min(da)
maxda = np.max(da)
daRange = maxda - minda;
for i in range(arrayShape[0]):
for j in range(arrayShape[1]):
if da[i, j] > minda + daRange*0.5:
# cstr = "k"
cstr = "w"
else:
# cstr = "w"
cstr = "k"
if np.abs(da[i,j]) < 100:
fsz = 9
else:
fsz = 6
if textOn:
if nData[(j,i)] > 0:
if forceInt:
ax.text(x[(j,i)]+dx/2, y[(j,i)]+dy/2, da[i, j].astype("int"),
ha="center", va="center", color=cstr, fontsize=fsz)
else:
ax.text(x[(j,i)]+dx/2, y[(j,i)]+dy/2, da[i, j],
ha="center", va="center", color=cstr, fontsize=fsz)
else:
ax.text(x[(j,i)]+dx/2, y[(j,i)]+dy/2, "-",
ha="center", va="center", color=cstr, fontsize=fsz)
ax.tick_params(axis = "both", labelsize = 12)
im_ratio = float(da.shape[0])/da.shape[1]
cbh = plt.colorbar(im,fraction=0.0477*im_ratio, pad=0.02)
cbh.ax.set_ylabel(colorBarLabel, fontSize = 16);
# ax.invert_yaxis();
In [ ]:
In this notebook we measure DR25 vetting completeness, defined as the fraction of detections (TCEs) that are correctly vetted as planet candidates. We use the set of injected on-target planets that were detected at the correct ephemeris as the base set of TCEs. All of these TCEs are "true planets" by definition. Then vetting completeness is the fraction of these TCEs that are vetter as PC by the robovetter. We study how vetting completeness depends on period and MES.
We think of TCEs as consisting of two sets: those that are dispositioned as FP and those that are dispositioned as PC. Then we can think of the vetting process as drawing from the set of TCEs, with a probability $r$ of selecting PCs. We identify $r$ with vetting completeness. Then the probability distribution of selecting $c$ FPs from $n$ TCEs is given by the binomial distribution
$$P\{c\} = \left( \begin{array}{c} n \\ c \end{array} \right) r^c (1-r)^{n-c}.$$In this spirit, we define the vetting effectiveness $r$ as the probability of drawing PCs from inverted/scrambled TCEs, found via the Bayesian inference $p(r|n, c) \propto p(c|r, n) p(r)$, where $c$ is the number of TCEs vetted as PCs, $n$ is the total number of TCEs, $$p(c|r, n) = \left( \begin{array}{c} n \\ c \end{array} \right) r^c (1-r)^{n-c}$$ and $p(r)$ is a prior distribution of the probability $r$. By putting the data on a grid indexed by $i,j$, we can fit effectiveness as a function parameterized by a vector $\theta$, $r(\theta,\mathrm{period},\mathrm{MES})$, as $p(\theta)|n_{i,j}, c_{i,j}, \mathrm{period}_{i,j},\mathrm{MES}_{i,j}) \propto p(c_{i,j}|\theta, n_{i,j}, \mathrm{period}_{i,j},\mathrm{MES}_{i,j}) p(\theta)$, where $p(\theta)$ is some prior distribution of the parameters.
First we define our stellar and planet populations.
In [3]:
stellarType = "GK"
scoreCut = 0.0;
scenario = "large"
if scenario == "small":
# small planet long period scenario
periodMin = 200;
periodMax = 400;
rpMin = 0.75;
rpMax = 2.5;
mesMin = 0;
mesMax = 30;
elif scenario == "large":
# all planet scenario
periodMin = 0;
periodMax = 500;
rpMin = 0.5;
rpMax = 15;
mesMin = 0;
mesMax = 30;
else:
raise ValueError('Bad scenario name');
Then we define our binomial probability distribution function.
In [4]:
def binPdf(n, r, c):
return sp.comb(n,c)*(r**c)*((1-r)**(n-c));
Then we define a bunch of models of the rate as functions of period ($x$) and MES ($y$) which are identified by the variable 'model'.
In [ ]:
Read in our data.
In [5]:
dataLoc = "../data/"
injTceList = dataLoc + "kplr_dr25_inj1_tces.txt"
tcelist = dataLoc + "DR25-Injected-Recovered-OnTarget-Planet-TCEs-1-1-Prat.txt"
# starlist = dataLoc + "dr25_stellar_updated_feh_" + stellarType + ".txt"
starlist = "../stellarCatalogs/dr25_stellar_supp_gaia_clean_" + stellarType + ".txt"
In [6]:
# Load the stellar population we want to use
kic = pd.read_csv(starlist)
# Load D2 table
injTces = ascii.read(injTceList)
tces = np.genfromtxt(tcelist, dtype='str')
tceKepids = np.zeros(len(tces));
for i in range(len(tces)):
s = tces[i].split('-');
tceKepids[i] = int(s[0]);
print(tceKepids)
print("num injected/recovered TCEs: " + str(np.size(tceKepids)))
print("num injected TCEs: " + str(np.size(injTces)))
In [7]:
injTces = injTces[np.in1d(injTces['TCE_ID'],tces)]
print("num injected TCEs after trimming to injected/recovered: " + str(np.size(injTces)))
In [8]:
# Select only those TCEs that are in this stellar population
injTces = injTces[np.in1d(injTces['KIC'],kic.kepid)]
print("after: " + str(np.size(injTces)))
In [9]:
# Do some basic stats
print(injTceList)
print("# of injected TCEs: " + str(len(injTces)))
print("# of injected PCs: " + str(len(injTces[injTces['Disp']=='PC'])))
print("# of injected FPs: " + str(len(injTces[injTces['Disp']=='FP'])))
print(' ')
print("for " + str(rpMax) + " < Rp < " + str(rpMax) + ", " + str(periodMin) + " < period < " + str(periodMax) + ":");
print("# of injected injected TCEs: " + str(len(injTces[np.all([ \
injTces['Rp']>rpMin,injTces['Rp']<rpMax,injTces['period']>periodMin,injTces['period']<periodMax], axis=0)])))
print("# of injected PCs: " + str(len(injTces[np.all([injTces['Disp']=='PC',\
injTces['Rp']>rpMin,injTces['Rp']<rpMax,injTces['period']>periodMin,injTces['period']<periodMax], axis=0)])))
print("# of injected FPs: " + str(len(injTces[np.all([injTces['Disp']=='FP',\
injTces['Rp']>rpMin,injTces['Rp']<rpMax,injTces['period']>periodMin,injTces['period']<periodMax], axis=0)])))
Separate out the PCs and FPs
In [10]:
pcIndex = np.where(injTces[injTces['Disp']=='PC'])
fpIndex = np.where(injTces[injTces['Disp']=='FP'])
pcs = injTces[pcIndex]
fps = injTces[fpIndex]
Select the TCEs that are in our desired population and plot them.
In [11]:
spIndex = np.where(np.all([
injTces['Rp']>rpMin,injTces['Rp']<rpMax,injTces['period']>periodMin,injTces['period']<periodMax], axis=0))
spInjTces = injTces[spIndex]
spInjPcs = spInjTces[(spInjTces['Disp']=='PC') & (spInjTces['Score']>=scoreCut)]
spInjFps = spInjTces[(spInjTces['Disp']=='FP') | (spInjTces['Score']<scoreCut)]
In [12]:
plt.figure(figsize=(15,15));
plt.subplot(2,2,1);
plt.scatter(injTces['period'], injTces['Expected_MES'], marker=".");
plt.ylim(0,mesMax);
plt.title("all injected TCEs");
plt.ylabel('Expected MES');
plt.xlabel('Period');
plt.subplot(2,2,2);
plt.scatter(spInjTces['period'], spInjTces['Expected_MES'], marker=".");
plt.ylim(0,mesMax);
plt.title("injected TCEs in period/MES range");
plt.xlabel('Period');
plt.ylabel('Expected MES');
plt.subplot(2,2,3);
plt.scatter(spInjPcs['period'], spInjPcs['Expected_MES'], marker=".");
plt.ylim(0,mesMax);
plt.title("injected PCs in period/MES range");
plt.ylabel('Expected MES');
plt.xlabel('Period');
plt.subplot(2,2,4);
plt.scatter(spInjFps['period'], spInjFps['Expected_MES'], marker=".");
plt.ylim(0,mesMax);
plt.title("injected FPss in period/MES range");
plt.ylabel('Expected MES');
plt.xlabel('Period');
Bin the populations onto a grid. The binned TCEs and PCs are the input to our MCMC analysis.
In [13]:
dPeriod = 10;
dMes = 1;
p0 = periodMin;
pEnd = periodMax;
m0 = mesMin;
mEnd = mesMax;
# make the period-mes grid
NPeriod = int((pEnd - p0)/dPeriod);
NMes = int((mEnd - m0)/dMes);
tceGrid = np.zeros((NPeriod,NMes));
cellPeriod = np.zeros((NPeriod,NMes));
cellMes = np.zeros((NPeriod,NMes));
pcGrid = np.zeros((NPeriod,NMes));
fpGrid = np.zeros((NPeriod,NMes));
# count how many points are in each cell
for p in range(NPeriod):
for m in range(NMes):
cellPeriod[(p,m)] = p0 + p*dPeriod;
cellMes[(p,m)] = m0 + m*dMes;
pointsInCell = np.where(
(spInjTces['period'] > cellPeriod[(p,m)])
& (spInjTces['period'] <= cellPeriod[(p,m)]+dPeriod)
& (spInjTces['Expected_MES'] > cellMes[(p,m)])
& (spInjTces['Expected_MES'] <= cellMes[(p,m)]+dMes));
tceGrid[(p,m)] = len(pointsInCell[0]);
pointsInCell = np.where(
(spInjPcs['period'] > cellPeriod[(p,m)])
& (spInjPcs['period'] <= cellPeriod[(p,m)]+dPeriod)
& (spInjPcs['Expected_MES'] > cellMes[(p,m)])
& (spInjPcs['Expected_MES'] <= cellMes[(p,m)]+dMes));
pcGrid[(p,m)] = len(pointsInCell[0]);
pointsInCell = np.where(
(spInjFps['period'] > cellPeriod[(p,m)])
& (spInjFps['period'] <= cellPeriod[(p,m)]+dPeriod)
& (spInjFps['Expected_MES'] > cellMes[(p,m)])
& (spInjFps['Expected_MES'] <= cellMes[(p,m)]+dMes));
fpGrid[(p,m)] = len(pointsInCell[0]);
In [14]:
drawHeatMap(tceGrid, (15,15), cellPeriod, cellMes, colorBarLabel="# of TCEs");
plt.ylabel('Expected MES', fontsize = 16);
plt.xlabel('Period', fontsize = 16);
plt.savefig("vetCompNTCEs.pdf",bbox_inches='tight')
plt.title("All Injected TCEs");
drawHeatMap(pcGrid, (15,15), cellPeriod, cellMes, colorBarLabel="# of PCs");
plt.title("Injected TCEs Dispositioned as PCs");
plt.ylabel('Expected MES', fontsize = 16);
plt.xlabel('Period', fontsize = 16);
drawHeatMap(fpGrid, (15,15), cellPeriod, cellMes, colorBarLabel="# of FPs");
plt.title("Injected TCEs Dispositioned as FPs");
plt.ylabel('Expected MES', fontsize = 16);
plt.xlabel('Period', fontsize = 16);
Compute the PC fraction in each cell. This is not used in our analysis, but is a qualitative guide suggesting what functions may be the best fit.
In [15]:
pcFrac = np.zeros(np.shape(tceGrid))
minTcePerCell = 0;
pcFrac[tceGrid>minTcePerCell] = pcGrid[tceGrid>minTcePerCell]/tceGrid[tceGrid>minTcePerCell];
drawHeatMap(np.round(100*pcFrac), (15,15), cellPeriod, cellMes, colorBarLabel="% PCs", nData = tceGrid);
plt.ylabel('Expected MES', fontsize = 16);
plt.xlabel('Period', fontsize = 16);
plt.savefig("vetCompInjRate.pdf",bbox_inches='tight')
plt.title("% of Injected TCEs Dispositioned as PCs", fontsize = 16);
pcFlat = pcGrid.flatten();
tceFlat = tceGrid.flatten();
# cellX = cellPeriod.flatten();
# cellY = cellMes.flatten();
# convert to homogeneous coordinates on unit square [0,1]
cellX, cellY = funcModels.normalizeRange(cellPeriod, cellMes, [periodMin, periodMax], [mesMin, mesMax]);
gridShape = np.shape(cellX);
dx = 1./gridShape[0];
dy = 1./gridShape[1];
print("gridShape = " + str(gridShape) + ", dx = " + str(dx) + ", dy = " + str(dy))
cellXFlat = cellX.flatten();
cellYFlat = cellY.flatten();
pcFlat[tceFlat<minTcePerCell] = 0;
tceFlat[tceFlat<minTcePerCell] = 0;
tceData = [cellXFlat, cellYFlat, tceFlat, pcFlat];
We're ready to compute a Bayesian inference of the success probability $r$:
$$p(r|c, n) \propto p(c|r, n) p(r).$$But we're computing $r$ as a function of period $p$, MES $m$, and parameters $\theta$, $r(\theta, p, m)$. So our inference becomes
$$p(\theta|c, n, p, m) \propto p(c|\theta, n, p, m) p(\theta).$$Because each cell is independent, we linearize the array to a list of cells indexed by $k$. Then the likelihood for each cell is
$$p(c_k|\theta, n_k, p_k, m_k) = \left( \begin{array}{c_k} n_k \\ c_k \end{array} \right) r(\theta, p_k , m_k )^{c_k} (1-r(\theta, p_k , m_k ))^{n_k-c_k}$$Because the $N$ cells are independent, the likelihood for the collection of cells is
$$p(c|\theta, n, p, m) \equiv p(c_1, \ldots, c_N|\theta, n_1, \ldots, n_N, p_1, \ldots, p_N, m_1, \ldots, m_N) = \prod_k \left( \begin{array}{c_k} n_k \\ c_k \end{array} \right) r(\theta, p_k , m_k )^{c_k} (1-r(\theta, p_k , m_k ))^{n_k-c_k}.$$The log-likelihood is then
$$\log p(c|\theta, n, p, m) = \sum_k \log \left(\left( \begin{array}{c_k} n_k \\ c_k \end{array} \right) r(\theta, p_k , m_k )^{c_k} (1-r(\theta, p_k , m_k ))^{n_k-c_k} \right)$$$$= \sum_k \left[ \log \left(\begin{array}{c_k} n_k \\ c_k \end{array} \right) + c_k \log \left(r(\theta, p_k , m_k ) \right) + \left( n_k-c_k \right) \log(1-r(\theta, p_k , m_k )) \right] $$
In [ ]:
We code this as
In [16]:
def lnBinlike(theta, data, model):
x, y, n, c = data;
r = funcModels.rateModel(x,y,theta,model);
clnr = c*np.log(r);
clnr[c==0] = 0;
lpl = np.sum(np.log(spec.comb(n,c)) + clnr + (n-c)*np.log(1-r));
# some diagnostics for when things go wrong
if np.isnan(lpl):
return -np.inf
else:
return lpl
For our prior $p(r)$, we'll set the prior = 1 on the interval $[0, 1]$ and zero otherwise.
In [17]:
def lnBinprior(theta, data, model):
x, y, n, c = data
# print(theta)
if model == "linearX":
if -5000.0 < theta[0] < 5000.0 and 0.0 < theta[1] < 1 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "linearXY":
if -5000.0 < theta[0] < 5000.0 and -5000.0 < theta[1] < 5000.0 \
and 0.0 < theta[2] < 1 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "gaussian":
if -10.0 < theta[0] < 10.0 and -10.0 < theta[1] < 10.0 \
and 1e-4 < theta[2] < 1e4 and 1e-4 < theta[3] < 1e4 and -1 <= theta[4] <= 1 and 0 <= theta[5] <= 1 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "logisticX":
if -10.0 < theta[0] < 10.0 \
and 1e-4 < theta[1] < 1e4 and 0 < theta[2] < 1e6 and 0 < theta[3] < 1e6 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "logisticX0":
if 0 <= theta[0] <= 1000 \
and 1e-4 < theta[1] < 1e4 and 0 < theta[2] < 1e6 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "logisticY0":
if -1 <= theta[0] <= 2 \
and 1e-4 < theta[1] < 1e4 and 0 < theta[2] < 1 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "logisticX0xlogisticY0":
if -1 <= theta[0] <= 2 and -1 <= theta[1] <= 2 \
and 1e-4 < theta[2] < 1e4 and 1e-4 < theta[3] < 1e4 \
and 0 < theta[4] < 1 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "logisticX0xlogisticY02":
if -1 <= theta[0] <= 2 and -1 <= theta[1] <= 2 \
and 1e-4 < theta[2] < 1e4 and 1e-4 < theta[3] < 1e4 \
and 0.01 < theta[4] < 10 and 0.01 < theta[5] < 10 \
and 0 < theta[6] < 1 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "logisticX0xRotatedLogisticY0":
if -1 <= theta[0] <= 2 and -1 <= theta[1] <= 2 \
and 1e-4 < theta[2] < 1e4 and 1e-4 < theta[3] < 1e4 \
and -180 < theta[4] < 180 \
and 0 < theta[5] < 1 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "logisticX0xRotatedLogisticY02":
if -1 <= theta[0] <= 2 and -1 <= theta[1] <= 2 \
and 1e-4 < theta[2] < 1e4 and 1e-4 < theta[3] < 1e4 \
and 0.01 < theta[4] < 10 \
and -180 < theta[5] < 180 \
and 0 < theta[6] < 1 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "rotatedLogisticX0xlogisticY0":
if -1 <= theta[0] <= 2 and -1 <= theta[1] <= 2 \
and 1e-4 < theta[2] < 1e4 and 1e-4 < theta[3] < 1e4 \
and -3 < theta[4] < 3 and -180 < theta[5] < 180 \
and 0 < theta[6] < 1 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "rotatedLogisticX0xlogisticY02":
if -1 <= theta[0] <= 2 and -1 <= theta[1] <= 2 \
and 1e-4 < theta[2] < 1e4 and 1e-4 < theta[3] < 1e4 \
and 0.01 < theta[4] < 10 and 0.01 < theta[5] < 10 \
and -180 < theta[6] < 180 and -180 < theta[7] < 180 \
and 0 < theta[8] < 1 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "rotatedLogisticX0":
if -1 <= theta[0] <= 2 \
and 1e-4 < theta[1] < 100 and 0 < theta[2] <= 1 and -180 < theta[3] < 180 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
elif model == "dualBrokenPowerLaw":
# print(funcModels.rateModel(x, y, theta, model))
if 0 <= theta[0] <= 1 and 0 <= theta[1] <= 1 \
and -2 < theta[2] < 0 and -2 < theta[3] < 0 and 0 < theta[4] < 1e4 and 0 < theta[5] < 1e4 \
and 0 < theta[6] < 1 \
and np.min(funcModels.rateModel(x, y, theta, model)) >= 0 \
and np.max(funcModels.rateModel(x, y, theta, model)) <= 1:
return 1.0
else:
raise ValueError('Bad model name');
# print(theta)
return -np.inf
Then the log posterior probability is $\log p(\theta|c, n, p, m) = \log p(c|\theta, n, p, m) + \log p(\theta)$, which we code as
In [18]:
def lnBinprob(theta, data, model):
lp = lnBinprior(theta, data, model)
# print("lnPoisprior = " + str(lp))
if not np.isfinite(lp):
return -np.inf
# print(str(lnPoislike(theta, A, c)))
return lp + lnBinlike(theta, data, model)
We now perform the MCMC calculation of the log posterior. We use a manual three-part strategy to find the best seed point: first we use the initial values in the model definitions. This MCMC result is used to seed the second iterations, whose result is used to seed the third and final iteration. We then initialize the MCMC walkers with a small Gaussian distribution around these starting points.
In [19]:
model = "rotatedLogisticX0xlogisticY02"
if model == "logisticY0":
initialPos = [ 0.14828331, 17.33408434, 0.92967224];
elif model == "logisticX0xlogisticY0":
initialPos = [ 0.99560747, 0.14886312, 4.89150268, 22.22093359, 0.94770438];
elif model == "logisticX0xlogisticY02":
initialPos = [ 0.81952689, 0.23524868, 4.7697679, 19.05683796, 2.05838984, 4.60039486, 0.99113786];
elif model == "rotatedLogisticX0xlogisticY0":
initialPos = [ 1.08006382, 0.14448152, 4.07613918, 15.42298136, 0.75826285, 7.55065579, 0.98498245];
elif model == "logisticX0xRotatedLogisticY0":
initialPos = [ 1.01211435, 0.14979708, 5.4723763, 13.37211524, 0, 0.98427409]
elif model == "logisticX0xRotatedLogisticY02":
initialPos = [ 1.01211435, 0.14979708, 5.4723763, 13.37211524, 5, 0, 0.98427409]
elif model == "rotatedLogisticX0xlogisticY02":
initialPos = [ 1.21729902, 0.25877038, 5.03162786, 21.4166877, 0.51381796, 4.01130569, 3.30628676, 6.15551683, 0.97623034];
elif model == "dualBrokenPowerLaw":
initialPos = [ 0.44265552, 0.3179024, -0.10705209, -0.98008117, 2.72776688, 0.06786803, 0.92982262];
else:
initialPos = funcModels.initRateModel(model);
print(initialPos)
In [20]:
import scipy.optimize as op
nll = lambda *args: -lnBinlike(*args)
result = op.minimize(nll, initialPos, args=(tceData, model))
maxLikelihoodResult = result["x"];
modelLabels = funcModels.getModelLabels(model)
for i in range(0,len(maxLikelihoodResult)):
print("maximum Likelihood " + modelLabels[i] + ":={:.3f}".format(maxLikelihoodResult[i]))
if lnBinprior(maxLikelihoodResult, tceData, model) == -np.inf:
maxLikelihoodResult = initialPos;
print("violates prior, replacing maxLikelihoodResult result with initialPos")
x, y, n, c = tceData
r = funcModels.rateModel(x,y,maxLikelihoodResult,model);
print("maximum Likelihood rate min = {:.3f}".format(np.min(np.min(r))) + ", max = {:.3f}".format(np.max(np.max(r))))
In [21]:
import emcee
ndim, nwalkers = len(maxLikelihoodResult), 100
pos = [maxLikelihoodResult + 1e-2*np.random.randn(ndim) for i in range(nwalkers)]
sampler = emcee.EnsembleSampler(nwalkers, ndim, lnBinprob, args=(tceData, model))
sampler.run_mcmc(pos, 5000);
samples = sampler.chain[:, 2000:, :].reshape((-1, ndim))
modelLabels = funcModels.getModelLabels(model)
dataResult = map(lambda v: (v[1], v[2]-v[1], v[1]-v[0]),
zip(*np.percentile(samples, [16, 50, 84], axis=0)))
dataResult = list(dataResult)
for i in range(0,ndim):
v = dataResult[i];
print("MCMC " + modelLabels[i] + ":={:.3f}".format(v[0]) + "+{:.3f}".format(v[1]) + "-{:.3f}".format(v[2]))
# print("true " + modelLabels[i] + ":={:.3f}".format(trueTheta[i]))
resultSize = np.shape(dataResult);
fitTheta = np.zeros(resultSize[0]);
for i in range(resultSize[0]):
fitTheta[i] = dataResult[i][0]
print("pcFitTheta:")
print(fitTheta)
modes = np.zeros(len(fitTheta))
for i in range(len(modes)):
modes[i] = stats.mode(np.round(samples[:,i], 4))[0]
print("modes:")
print(modes)
# print("compared to: rate={:.3f}".format(rate))
In [22]:
reload(funcModels)
plt.figure(figsize=(10,5))
for i in range(0,ndim):
plt.subplot(ndim,1,i+1)
plt.plot(np.transpose(sampler.chain[:, :, i]), color="k", alpha=0.1);
plt.ylabel(modelLabels[i]);
import corner
modelLabels = funcModels.getModelLabels(model)
# fig = corner.corner(samples, labels=["$m$", "$b$", "$\ln\,f$"],
# truths=[m_true, b_true, np.log(f_true)])
fig = corner.corner(samples, labels = modelLabels, label_kwargs = {"fontsize": 32}, truths = fitTheta)
plt.savefig("vetCompPost.pdf",bbox_inches='tight')
In [ ]:
We test the result by reconstructing the distribution of PCs and % of PCs using binomial-distributed random numbers, to see if they match the actual data.
In [23]:
fitGrid = np.zeros(np.shape(tceGrid));
resultSize = np.shape(dataResult);
fitTheta = np.zeros(resultSize[0]);
for i in range(resultSize[0]):
fitTheta[i] = dataResult[i][0]
print("fitTheta = " + str(fitTheta))
for p in range(NPeriod):
for m in range(NMes):
fitGrid[(p,m)] = np.random.binomial(tceGrid[(p,m)],
funcModels.rateModel(cellX[(p,m)]+dx/2, cellY[(p,m)]+dy/2, fitTheta, model), 1);
drawHeatMap(fitGrid, (15,15), cellPeriod, cellMes, nData = tceGrid);
plt.title("Simulated TCEs Dispositioned as PCs");
plt.ylabel('Expected MES');
plt.xlabel('Period');
fitFrac = np.zeros(np.shape(tceGrid))
fitFrac[tceGrid>minTcePerCell] = fitGrid[tceGrid>minTcePerCell]/tceGrid[tceGrid>minTcePerCell];
drawHeatMap(np.round(100*fitFrac), (15,15), cellPeriod, cellMes, nData = tceGrid);
plt.title("Simulated % of TCEs Dispositioned as PCs");
plt.ylabel('Expected MES');
plt.xlabel('Period');
Now do many realizations, and subtract the average from the observed to look for systematic differences.
In [ ]:
In [24]:
nFits = 1000;
fitGrid = np.zeros([np.shape(tceGrid)[0],np.shape(tceGrid)[1],nFits]);
sidx = [0]*nFits
progress = FloatProgress(min=0, max=nFits)
display(progress)
for f in range(nFits):
sidx[f] = int(np.random.uniform(high=samples.shape[0]-1));
tTheta = samples[sidx[f],:]
for p in range(NPeriod):
for m in range(NMes):
rm = funcModels.rateModel(cellX[(p,m)]+dx/2, cellY[(p,m)]+dy/2, tTheta, model)
if rm > 1:
rm = 1;
fitGrid[(p,m,f)] = np.random.binomial(tceGrid[(p,m)], rm, 1);
progress.value += 1
meanFit = np.mean(fitGrid, 2)
stdFit = np.std(fitGrid, 2)
In [25]:
drawHeatMap(meanFit, (15,15), cellPeriod, cellMes, nData = tceGrid);
plt.title("Mean Number of Simulated TCEs Dispositioned as PCs");
plt.ylabel('Expected MES');
plt.xlabel('Period');
fitFracMean = np.zeros(np.shape(tceGrid))
fitFracMean[tceGrid>minTcePerCell] = meanFit[tceGrid>minTcePerCell]/tceGrid[tceGrid>minTcePerCell];
drawHeatMap(np.round(100*fitFracMean), (15,15), cellPeriod, cellMes, nData = tceGrid, colorBarLabel="Mean PC %");
plt.ylabel('Expected MES', fontsize = 16);
plt.xlabel('Period', fontsize = 16);
plt.savefig("vetCompMean.pdf",bbox_inches='tight')
plt.title("Mean Simulated % of TCEs Dispositioned as PCs");
fitFracStd = np.zeros(np.shape(tceGrid))
fitFracStd[tceGrid>minTcePerCell] = stdFit[tceGrid>minTcePerCell]/tceGrid[tceGrid>minTcePerCell];
drawHeatMap(np.round(100*fitFracStd), (15,15), cellPeriod, cellMes, nData = tceGrid, colorBarLabel="Standard Deviation %");
plt.ylabel('Expected MES', fontsize = 16);
plt.xlabel('Period', fontsize = 16);
plt.savefig("vetCompStd.pdf",bbox_inches='tight')
plt.title("Standard Deviation of the Simulated % of TCEs Dispositioned as PCs");
In [26]:
drawHeatMap(np.round(100*pcFrac), (15,15), cellPeriod, cellMes, nData = tceGrid);
plt.title("Fraction of TCEs Dispositioned as PCs");
plt.ylabel('Expected MES');
plt.xlabel('Period');
In [ ]:
In [ ]:
In [27]:
fitDiff = fitFracMean - pcFrac
fitDiffNorm =np.zeros(fitDiff.shape)
fitDiffNorm[tceGrid>minTcePerCell] = fitDiff[tceGrid>minTcePerCell]/stdFit[tceGrid>minTcePerCell];
drawHeatMap(np.round(100*fitDiff), (15,15), cellPeriod, cellMes, nData = tceGrid);
plt.title("Residual from mean");
plt.ylabel('Expected MES');
plt.xlabel('Period');
drawHeatMap(np.round(fitDiffNorm), (15,15), cellPeriod, cellMes, nData = tceGrid,
colorBarLabel="Mean Residual ($\sigma$)");
plt.ylabel('Expected MES', fontsize = 16);
plt.xlabel('Period', fontsize = 16);
plt.savefig("vetCompMeanResid.pdf",bbox_inches='tight')
plt.title("Residual from mean (standard deviations)");
plt.figure(figsize=(15,5));
plt.hist(fitDiffNorm.flatten()[tceFlat > 0], 100);
np.median(fitDiffNorm.flatten()[tceFlat > 0])
Out[27]:
In [28]:
def binPdf(n, r, c):
return spec.comb(n,c)*(r**c)*((1-r)**(n-c));
def plot_norm_bin(n, r, scale):
xx = np.arange(0, n, 0.01)
ix = np.arange(0, n)
plt.plot(xx/n - r,scale*binPdf(n,r,xx)/max(binPdf(n,r,xx)));
residuals = np.zeros(tceGrid.shape);
rateGrid = np.zeros(tceGrid.shape);
for p in range(NPeriod):
for m in range(NMes):
rateGrid[(p,m)] = funcModels.rateModel(cellX[(p,m)]+dx/2, cellY[(p,m)]+dy/2, fitTheta, model);
if tceGrid[(p,m)] > 0:
residuals[(p,m)] = pcGrid[(p,m)]/tceGrid[(p,m)] - rateGrid[(p,m)]
rateFlat = rateGrid.flatten();
residualsFlat = residuals.flatten();
# group residuals by rate
plt.figure(figsize=(15,5));
histVals = plt.hist(residualsFlat[(rateFlat>0.9)&(tceFlat>0)], 35);
tcePctiles = np.percentile(tceFlat[(rateFlat>0.9)&(tceFlat>0)], [10, 50, 90], axis=0);
plot_norm_bin(np.mean(tceFlat[(rateFlat>0.9)&(tceFlat>0)]), 0.95, np.max(histVals[0]))
plot_norm_bin(tcePctiles[0], 0.95, np.max(histVals[0]))
plot_norm_bin(tcePctiles[1], 0.95, np.max(histVals[0]))
plot_norm_bin(tcePctiles[2], 0.95, np.max(histVals[0]))
plt.grid(linestyle = ':');
histVals = plt.figure(figsize=(15,5));
histVals = plt.hist(residualsFlat[(rateFlat>0.2)&(rateFlat<0.8)&(tceFlat>0)], 20);
tcePctiles = np.percentile(tceFlat[(rateFlat>0.9)&(tceFlat>0)], [10, 50, 90], axis=0);
plot_norm_bin(np.mean(tceFlat[(rateFlat>0.2)&(rateFlat<0.8)&(tceFlat>0)]), 0.5, np.max(histVals[0]))
plot_norm_bin(tcePctiles[0], 0.5, np.max(histVals[0]))
plot_norm_bin(tcePctiles[1], 0.5, np.max(histVals[0]))
plot_norm_bin(tcePctiles[2], 0.5, np.max(histVals[0]))
plt.grid(linestyle = ':');
In [29]:
np.percentile(tceFlat[(rateFlat>0.9)&(tceFlat>0)], [10, 50, 90], axis=0)
Out[29]:
Plot the fitted functional form of the vetting efficiency.
In [30]:
from mpl_toolkits.mplot3d import Axes3D # noqa: F401 unused import
from matplotlib import cm
Z = funcModels.rateModel(cellX, cellY, fitTheta, model);
fig = plt.figure(figsize=plt.figaspect(0.3));
ax = fig.add_subplot(1, 3, 1, projection='3d')
surf = ax.plot_surface(cellPeriod, cellMes, Z, alpha = 0.5);
scat = ax.scatter(cellPeriod[tceGrid>0], cellMes[tceGrid>0], pcFrac[tceGrid>0], c='r', marker = '.');
plt.xlabel("period");
plt.ylabel("Expected MES");
ax.view_init(0,0)
ax = fig.add_subplot(1, 3, 2, projection='3d')
surf = ax.plot_surface(cellPeriod, cellMes, Z, alpha = 0.5);
scat = ax.scatter(cellPeriod[tceGrid>0], cellMes[tceGrid>0], pcFrac[tceGrid>0], c='r', marker = '.');
plt.xlabel("period");
plt.ylabel("Expected MES");
ax.view_init(0,-90)
plt.title("Vetting completeness");
ax = fig.add_subplot(1, 3, 3, projection='3d')
ax = fig.gca(projection='3d')
surf = ax.plot_surface(cellPeriod, cellMes, Z, alpha = 0.5);
scat = ax.scatter(cellPeriod[tceGrid>0], cellMes[tceGrid>0], pcFrac[tceGrid>0], c='r', marker = '.');
plt.xlabel("period");
plt.ylabel("Expected MES");
fig, ax = plt.subplots(figsize=(15,10));
CS = ax.contour(cellPeriod, cellMes, Z, colors='k', levels = [0, .1, .2, .3, .4, .5, .6, .7, .8, .9, .95, .96, .97, .98, .99]);
ax.clabel(CS, inline=1, fontsize=18);
scf = ax.scatter(cellPeriod[tceGrid>0], cellMes[tceGrid>0], cmap="cividis", c=pcFrac[tceGrid>0], s=5*tceGrid[tceGrid>0], alpha = 0.5);
plt.xlabel("period", fontSize = 24);
plt.ylabel("Expected MES", fontSize = 24);
cbh = plt.colorbar(scf);
cbh.ax.set_ylabel("Measured Fraction");
plt.tick_params(labelsize = 12)
plt.savefig("vetCompContours.pdf",bbox_inches='tight')
plt.title("Vetting completeness. Size of marker = # of TCEs in cell", fontSize = 24);
In [31]:
sp = np.zeros([3,3])
sPeriod = np.array([[0, 10, 200], [0, 10, 200], [0, 10, 200]])
sMes = np.array([[0, 0, 0], [10, 10, 10], [30, 30, 30]])
sp[0,0] = np.mean(np.mean(Z[np.where((cellPeriod > 0) & (cellPeriod <= 10) & (cellMes > 20) & (cellMes <= 200))]))
sp[0,1] = np.mean(np.mean(Z[np.where((cellPeriod > 10) & (cellPeriod <= 200) & (cellMes > 20) & (cellMes <= 200))]))
sp[0,2] = np.mean(np.mean(Z[np.where((cellPeriod > 200) & (cellPeriod <= 500) & (cellMes > 20) & (cellMes <= 200))]))
sp[1,0] = np.mean(np.mean(Z[np.where((cellPeriod > 0) & (cellPeriod <= 10) & (cellMes > 10) & (cellMes <= 20))]))
sp[1,1] = np.mean(np.mean(Z[np.where((cellPeriod > 10) & (cellPeriod <= 200) & (cellMes > 10) & (cellMes <= 20))]))
sp[1,2] = np.mean(np.mean(Z[np.where((cellPeriod > 200) & (cellPeriod <= 500) & (cellMes > 10) & (cellMes <= 20))]))
sp[2,0] = np.mean(np.mean(Z[np.where((cellPeriod > 0) & (cellPeriod <= 10) & (cellMes > 0) & (cellMes <= 10))]))
sp[2,1] = np.mean(np.mean(Z[np.where((cellPeriod > 10) & (cellPeriod <= 200) & (cellMes > 0) & (cellMes <= 10))]))
sp[2,2] = np.mean(np.mean(Z[np.where((cellPeriod > 200) & (cellPeriod <= 500) & (cellMes > 0) & (cellMes <= 10))]))
xp = np.array([[0, 1, 2], [0, 1, 2], [0, 1, 2]])
yp = np.array([[0, 0, 0], [1, 1, 1], [2, 2, 2]])
dxp = 1
dyp = 1
imageSize = (3,3)
plt.figure(figsize=imageSize);
fig, ax = plt.subplots(figsize=imageSize);
da = np.transpose(sp);
ax.imshow(da);
# ax.imshow(da, origin='lower');
arrayShape = da.shape;
for i in range(arrayShape[0]):
for j in range(arrayShape[1]):
if da[i, j] < 0.85:
co = "w"
else:
co = "k"
text = ax.text(xp[(j,i)]+dxp/2, yp[(j,i)]+dyp/2, round(da[i, j],3),
ha="center", va="center", color=co);
sp
Out[31]:
In [ ]:
In [ ]:
In [32]:
r1 = np.zeros(np.shape(samples)[0])
xp = 50.;
yp = 25.;
cx = (xp - periodMin)/(periodMax - periodMin);
cy = (yp - mesMin)/(mesMax - mesMin);
for i in range(np.shape(samples)[0]):
r1[i] = funcModels.rateModel(cx, cy, samples[i,:], model)
f1 = funcModels.rateModel(cx, cy, fitTheta, model)
r2 = np.zeros(np.shape(samples)[0])
xp = 365.;
yp = 10.;
cx = (xp - periodMin)/(periodMax - periodMin);
cy = (yp - mesMin)/(mesMax - mesMin);
for i in range(np.shape(samples)[0]):
r2[i] = funcModels.rateModel(cx, cy, samples[i,:], model)
f2 = funcModels.rateModel(cx, cy, fitTheta, model)
In [33]:
greyLevel = "0.7"
rr = np.percentile(r1, [5, 95]);
plt.hist(r1[(r1 > 0.95*rr[0]) & (r1 < 1.05*rr[1])], 100, color=greyLevel);
plt.plot([f1, f1], [0, 3000], color='k', linestyle='--', linewidth=1)
rr = np.percentile(r2, [5, 95]);
plt.hist(r2[(r2 > 0.95*rr[0]) & (r2 < 1.05*rr[1])], 100, color=greyLevel);
plt.plot([f2, f2], [0, 3000], color='k', linestyle='--', linewidth=1)
plt.xlabel("Vetting Completeness")
plt.savefig("vetCompExamples.pdf",bbox_inches='tight')
In [34]:
np.percentile(r1, [16, 50, 84])
Out[34]:
In [35]:
np.percentile(r2, [16, 50, 84])
Out[35]:
In [ ]:
In [36]:
l = np.zeros(np.shape(samples)[0])
aicDist = np.zeros(np.shape(samples)[0])
progress = FloatProgress(min=0, max=samples.shape[0])
display(progress)
for i in range(samples.shape[0]):
l[i] = lnBinprob(samples[i,:], tceData, model)
aicDist[i] = 2*len(samples[i,:]) - 2*lnBinlike(samples[i,:], tceData, model)
progress.value += 1
In [37]:
l[l<-1e8] = -1e8;
aicDist[aicDist>1e8] = 1e8;
minAic = np.min(aicDist)
In [38]:
plt.hist(aicDist[aicDist<1e8], 100);
In [39]:
samples[np.argmin(aicDist),:]
Out[39]:
In [40]:
fitTheta
Out[40]:
In [41]:
2*len(fitTheta) - 2*lnBinlike(samples[np.argmin(aicDist),:], tceData, model)
Out[41]:
In [42]:
plt.hist(l[l>-1e8] - np.median(l[l>-1e8]), 100);
In [43]:
plt.hist(np.exp(l[l>-1e8] - np.median(l[l>-1e8])), 100);
In [44]:
np.median(l[l>-1e8])
Out[44]:
In [45]:
aic = 2*len(fitTheta) - 2*(lnBinlike(fitTheta, tceData, model))
aic
Out[45]:
In [46]:
maxLikelihoodAic = 2*len(maxLikelihoodResult) - 2*lnBinlike(maxLikelihoodResult, tceData, model)
maxLikelihoodAic
Out[46]:
In [ ]:
In [ ]:
In [47]:
from skmonaco import mcquad
lbnds = np.empty([np.shape(samples)[1]])
ubnds = np.empty([np.shape(samples)[1]])
for i in range(len(lbnds)):
lbnds[i] = np.min(samples[:,i])
ubnds[i] = np.max(samples[:,i])
regularizationOffset = np.median(l)
def linBinProbInt(theta):
return np.exp(lnBinprob(theta, tceData, model) - regularizationOffset)
BF, BFerror = mcquad(linBinProbInt, xl=lbnds,xu=ubnds, npoints=1e7,nprocs=8 )
print("BF = {:.3e} +/- {:.3e}").format(BF,BFerror)
In [ ]:
In [ ]:
In [ ]:
In [ ]:
In [48]:
Z = funcModels.evaluateModel(cellPeriod, cellMes, fitTheta, [periodMin, periodMax], [mesMin, mesMax], model);
fig, ax = plt.subplots(figsize=(15,10));
CS = ax.contour(cellPeriod, cellMes, Z, colors='k', levels = [0, .1, .2, .3, .4, .5, .6, .7, .8, .9, .95, .96, .97, .98, .99]);
ax.clabel(CS, inline=1, fontsize=10);
scf = ax.scatter(cellPeriod[tceGrid>0], cellMes[tceGrid>0], cmap="cividis", c=pcFrac[tceGrid>0], s=5*tceGrid[tceGrid>0], alpha = 0.5);
plt.xlabel("period");
plt.ylabel("Expected MES");
plt.title("Vetting completeness. Size of marker = # of TCEs in cell");
cbh = plt.colorbar(scf);
cbh.ax.set_ylabel("Measured Rate");
We perform Bayesian model comparison by computing the Bayes factor
$$ \frac{P(D|M_2)}{P(D|M_1)} = \frac{\int P(D|\theta, M_2)P(\theta| M_2) d\theta}{\int P(D|\theta, M_1)P(\theta| M_1) d\theta} = \frac{\int \mathrm{Post}(\theta, M_2) d\theta}{\int \mathrm{Post}(\theta, M_1) d\theta},$$the integral of the posterior distribution. Because the posteriors are given as log posteriors, $\mathrm{Post}(\theta, M_1) = \exp (\mathrm{logPost}(\theta, M_1))$
Because the log likelihoods are large and negative, we run into precision problems when we exponentiate. We sddress this by, for each model, subtracting $c_k = \mathrm{median}(\mathrm{logPost}(\theta, M_k))$ in the exponential. Then, setting $f_k(\theta) = \mathrm{logPost}(\theta, M_k)$,
$$ \frac{\int \mathrm{Post}(\theta, M_2) d\theta}{\int \mathrm{Post}(\theta, M_1) d\theta} = \frac{\int e^{f_2(\theta)} d\theta}{\int e^{f_1(\theta)} d\theta} = e^{c_2-c_1}\frac{\int e^{f_2(\theta) - c_2} d\theta}{\int e^{f_1(\theta) - c_1} d\theta}$$In [49]:
import os.path
import pickle
fname = "vetCompletenessTable.pkl"
if os.path.isfile(fname):
modelComparisonTable = pd.read_pickle(fname)
else:
modelComparisonTable = pd.DataFrame({"Model": ["logisticY0", "dualBrokenPowerLaw",
"logisticX0xlogisticY0", "logisticX0xlogisticY02",
"logisticX0xRotatedLogisticY0", "logisticX0xRotatedLogisticY02",
"rotatedLogisticX0xlogisticY0", "rotatedLogisticX0xlogisticY02" ],
"medianMCMCAIC": [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
"minMCMCAIC": [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
"maxLikelihoodAIC": [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
"MedianLogPost": [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
"IntegralPost": [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
"IntegralPostErr": [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
"medianMCMCTheta": [[0],[0],[0],[0],[0],[0],[0],[0]],
"maxLikelihoodTheta": [[0],[0],[0],[0],[0],[0],[0],[0]],
"periodRange": [[0],[0],[0],[0],[0],[0],[0],[0]],
"mesRange": [[0],[0],[0],[0],[0],[0],[0],[0]]},
columns=["Model","BayesFactor","BayesFactorError","AICRelativeProb","medianMCMCAIC",
"minMCMCAIC","maxLikelihoodAIC",
"IntegralPost","IntegralPostErr","MedianLogPost","medianMCMCTheta",
"maxLikelihoodTheta","periodRange","mesRange"])
modelComparisonTable['IntegralPost'] = modelComparisonTable['IntegralPost'].map('{:,.3e}'.format)
modelComparisonTable['IntegralPostErr'] = modelComparisonTable['IntegralPostErr'].map('{:,.3e}'.format)
In [ ]:
In [50]:
mctIndex = np.where(modelComparisonTable["Model"].isin([model]))[0][0]
print(mctIndex)
modelComparisonTable["medianMCMCAIC"][mctIndex] = aic;
modelComparisonTable["minMCMCAIC"][mctIndex] = minAic;
modelComparisonTable["maxLikelihoodAIC"][mctIndex] = maxLikelihoodAic;
modelComparisonTable["MedianLogPost"][mctIndex] = regularizationOffset;
modelComparisonTable["IntegralPost"][mctIndex] = BF;
modelComparisonTable["IntegralPostErr"][mctIndex] = BFerror;
modelComparisonTable["medianMCMCTheta"][mctIndex] = fitTheta;
modelComparisonTable["maxLikelihoodTheta"][mctIndex] = maxLikelihoodResult;
modelComparisonTable["periodRange"][mctIndex] = [periodMin, periodMax];
modelComparisonTable["mesRange"][mctIndex] = [mesMin, mesMax];
We also compute the relative probability from the $\mathrm{AIC} = 2k - 2 \log(\mathrm{likelihood})$, where $k$ is the number of parameters in the model and the relative probability is $\exp\left(\left(\mathrm{AIC}_\mathrm{min} - \mathrm{AIC}\right)/2\right)$.
In [51]:
modelToCompareIndex = 5
modelComparisonTable["AICRelativeProb"] = 0.
minAic = np.min(modelComparisonTable["medianMCMCAIC"][modelToCompareIndex])
for i in range(len(modelComparisonTable)):
modelComparisonTable["AICRelativeProb"].iloc[i] = np.exp((minAic - modelComparisonTable["medianMCMCAIC"].iloc[i])/2.)
In [52]:
modelComparisonTable["BayesFactor"] = 0.
c1 = modelComparisonTable["MedianLogPost"].iloc[modelToCompareIndex]
i1 = np.double(modelComparisonTable["IntegralPost"].iloc[modelToCompareIndex])
for i in range(len(modelComparisonTable)):
c2 = modelComparisonTable["MedianLogPost"].iloc[i]
modelComparisonTable["BayesFactor"].iloc[i] = np.exp(c2 - c1)*np.double(modelComparisonTable["IntegralPost"].iloc[i])/i1
Because the terms in the Bayes factor are computed via Monte Carlo integration with a non-trivial error, we propagate that error through to an error on the Bayes factor.
In [53]:
modelComparisonTable["BayesFactorError"] = 0.
B = np.double(modelComparisonTable["IntegralPost"].iloc[modelToCompareIndex])
sB = np.double(modelComparisonTable["IntegralPostErr"].iloc[modelToCompareIndex])
c1 = modelComparisonTable["MedianLogPost"].iloc[modelToCompareIndex]
for i in range(len(modelComparisonTable)):
c2 = modelComparisonTable["MedianLogPost"].iloc[i]
f = np.double(modelComparisonTable["BayesFactor"].iloc[i])
A = np.exp(c2 - c1)*np.double(modelComparisonTable["IntegralPost"].iloc[i])
sA = np.exp(c2 - c1)*np.double(modelComparisonTable["IntegralPostErr"].iloc[i])
modelComparisonTable["BayesFactorError"].iloc[i] = f*np.sqrt((sA/A)**2 + (sB/B)**2)
In [54]:
modelComparisonTable
Out[54]:
In [55]:
modelComparisonTable.to_pickle(fname)
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tt = pd.read_pickle(fname)
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In [57]:
tt
Out[57]:
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%%javascript
IPython.notebook.save_notebook()
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%%bash -s "$model"
jupyter nbconvert --to html binomialVettingCompleteness.ipynb
mv binomialVettingCompleteness.html htmlArchive/binomialVettingCompleteness_$1.html
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injTces
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tces
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